Observations of the sodium layer using a Fabry-Perot spectrometer - Twilight temperature variations

Details Observations of the sodium layer using a Fabry-Perot spectrometer - Twilight temperature variations Observations of the sodium layer using a Fabry-Perot spectrometer - Twilight temperature variations

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jatp...51...91g&link_type=abstract

Journal of Atmospheric and Terrestrial Physics (ISSN 0021-9169), vol. 51, Feb. 1989, p. 91-99.

Physics

5

Atmospheric Temperature, Emission Spectra, Midlatitude Atmosphere, Sodium, Temperature Measurement, Fabry-Perot Spectrometers, Temperature Distribution, Twilight Glow

Scientific paper

Observations of the twilight Na emission from the 90-km level have been made at Mt. Torrens, a southern midlatitude station, using a high resolution Fabry-Perot spectrometer. An outline of the analysis required to determine temperatures is presented. A winter mean temperature of 199 K and a summer mean temperature of 150 K are determined from 2 years of data. The diurnal tide is shown to produce a distinct difference between the dawn and dusk temperatures during late summer and autumn.

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